LFAST- Large Fiber Array Spectroscopic Telescope: Prime Focus Corrector Optics

Andy Monson, Joel Berkson, Chad Bender, Roger Angel, Peter Gray, Kevin Gilliam, Chistian Schwab, Warren Foster

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The Large Fiber Array Spectroscopic Telescope (LFAST) is designed to be a cost-efficient way to provide a large collecting area for spectroscopy by duplicating large numbers of small (0.76m f/3.33) spherical mirror 'unit' telescopes. Each telescope is equipped with a prime focus corrector (PFC) feeding a guider and an optical fiber; and all the fiber optics will feed into a large spectrograph. The design of the PFC is driven by the need to minimize costs while achieving acceptable performance. We are currently constructing a prototype 20-unit system for testing in the second half of 2024. For this 20-unit system we have begun coordinating with industry about scaling for mass fabrication. In this paper we will present status updates from the performance of this early version of the prime focus corrector.

Original languageEnglish (US)
Title of host publicationGround-Based and Airborne Telescopes X
EditorsHeather K. Marshall, Jason Spyromilio, Tomonori Usuda
PublisherSPIE
ISBN (Electronic)9781510675117
DOIs
StatePublished - 2024
EventGround-Based and Airborne Telescopes X 2024 - Yokohama, Japan
Duration: Jun 16 2024Jun 21 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13094
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceGround-Based and Airborne Telescopes X 2024
Country/TerritoryJapan
CityYokohama
Period6/16/246/21/24

Keywords

  • Array Telescope
  • LFAST
  • Optomechanical Design

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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